Eratosthenian

{{short description|Lunar geologic period}}

{{More references|date=December 2009}}

{{Infobox geologic timespan

| name = Eratosthenian

| manual_color = rgb(60.0, 213.0, 185.0)

| top_bar = Lunar

| time_start = 3200

| time_end = 1100

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| timeline = Lunar periods

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| celestial_body = moon

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| timescales_used = Lunar Geologic Timescale

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The Eratosthenian period in the lunar geologic timescale runs from 3,200 million years ago to 1,100 million years ago. It is named after the crater Eratosthenes, which displays characteristics typical of craters of this age, including a surface that is not significantly eroded by subsequent impacts, but which also does not possess a ray system. The massive basaltic volcanism of the Imbrian period tapered off and ceased during this long span of lunar time. The youngest lunar lava flows identified from orbital images are tentatively placed near the end of this period.

Its equivalent on Earth consists of most of the Mesoarchean and Neoarchean eras (Archean eon), Paleoproterozoic and Mesoproterozoic eras (Proterozoic eon).

Examples

Other than Eratosthenes itself, examples of large Eratosthenian craters on the near side of the Moon include Langrenus, Macrobius, Aristoteles, Hausen, Moretus, Pythagoras, Scoresby, Bullialdus, Plutarch, and Cavalerius. On the far side, examples include Olcott, Hamilton, Birkeland, Finsen, Kirkwood, and Ricco.[https://www.lpi.usra.edu/resources/mapcatalog/UGM/ Unified Geologic Map of the Moon], C. M. Fortezzo, P. D. Spudis, S. L. Harrel, 2020. United States Geological Survey.

File:Eratosthenes (LRO).png|Eratosthenes

File:Macrobius crater AS17-M-0296.jpg|Macrobius

File:Hausen crater 4193 h2.jpg|Hausen

File:Olcott crater AS16-M-3001 ASU.jpg|Olcott

File:Kirkwood crater 5029 h3.jpg|Kirkwood

References

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{{Timeline_Lunar_Geological_Timescale}}

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